Comment on: A SuperMassive Black Hole Fundamental Plane for Ellipticals

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dc.creatorGraham, Alister W.
dc.date2007-05-24
dc.date.accessioned2026-07-07T08:03:04Z
dc.date.available2026-07-07T08:03:04Z
dc.descriptionA simple regression analysis designed for predicting the supermassive black hole mass from the effective radius and mean effective surface brightness of the host bulge has been performed using the data from Barway & Kembhavi (arXiv:0705.1508). The scatter in the log M_bh direction is 0.32 dex, greater than reported and comparable with values obtained using a single predictor quantity such as luminosity, velocity dispersion or Sersic index.
dc.description2 page research note
dc.identifierhttps://arxiv.org/abs/0705.3509
dc.identifierhttp://arxiv.org/abs/0705.3509
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/129444
dc.subjectAstrophysics
dc.titleComment on: A SuperMassive Black Hole Fundamental Plane for Ellipticals
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